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Cody Messick

Researcher at Pennsylvania State University

Publications -  103
Citations -  47088

Cody Messick is an academic researcher from Pennsylvania State University. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 53, co-authored 84 publications receiving 38739 citations. Previous affiliations of Cody Messick include University of Texas at Austin.

Papers
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Journal ArticleDOI

GW150914: implications for the stochastic gravitational wave background from binary black holes

B. P. Abbott, +956 more
TL;DR: It is concluded that the stochastic gravitational-wave background from binary black holes, created from the incoherent superposition of all the merging binaries in the Universe, is potentially measurable by the Advanced LIGO and Advanced Virgo detectors operating at their projected final sensitivity.
Journal ArticleDOI

Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914

B. P. Abbott, +1002 more
TL;DR: The transient noise backgrounds used to determine the significance of the event (designated GW150914) are described and the results of investigations into potential correlated or uncorrelated sources of transient noise in the detectors around the time of theevent are presented.
Journal ArticleDOI

Localization and broadband follow-up of the gravitational-wave transient GW150914

B. P. Abbott, +1622 more
TL;DR: In this article, the sky localization of the first observed compact binary merger is presented, where the authors describe the low-latency analysis of the LIGO data and present a sky localization map.
Journal ArticleDOI

Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run

B. P. Abbott, +1067 more
TL;DR: This work performs a search for the isotropic stochastic gravitational-wave background using data from Advanced Laser Interferometer Gravitational Wave Observatory's (aLIGO) first observing run, and constrain the dimensionless energy density of gravitational waves to be Ω_{0}<1.7×10^{-7} with 95% confidence.